In astronomy, Kepler's laws of planetary motion, published by Johannes Kepler between 1609 and 1619, describe the orbits of planets around the Sun. The laws modified the heliocentric theory of Nicolaus Copernicus, replacing its circular orbits and epicycles with elliptical trajectories, and explaining how planetary velocities vary. The three laws state that:
In astronomy, Kepler's laws of planetary motion, published by Johannes Kepler between 1609 and 1619, describe the orbits of planets around the Sun. The laws modified the heliocentric theory of Nicolaus Copernicus, replacing its circular orbits and epicycles with elliptical trajectories, and explaining how planetary velocities vary. The three laws state that:1.The orbit of a planet is an ellipse with the Sun at one of the two foci.
In astronomy, Kepler's laws of planetary motion, published by Johannes Kepler between 1609 and 1619, describe the orbits of planets around the Sun. The laws modified the heliocentric theory of Nicolaus Copernicus, replacing its circular orbits and epicycles with elliptical trajectories, and explaining how planetary velocities vary. The three laws state that:1.The orbit of a planet is an ellipse with the Sun at one of the two foci.2.A line segment joining a planet and the Sun sweeps out equal areas during equal intervals of time.
In astronomy, Kepler's laws of planetary motion, published by Johannes Kepler between 1609 and 1619, describe the orbits of planets around the Sun. The laws modified the heliocentric theory of Nicolaus Copernicus, replacing its circular orbits and epicycles with elliptical trajectories, and explaining how planetary velocities vary. The three laws state that:1.The orbit of a planet is an ellipse with the Sun at one of the two foci.2.A line segment joining a planet and the Sun sweeps out equal areas during equal intervals of time.3. The square of a planet's orbital period is proportional to the cube of the length of the semi-major axis of its orbit.
Answers & Comments
Explanation:
In astronomy, Kepler's laws of planetary motion, published by Johannes Kepler between 1609 and 1619, describe the orbits of planets around the Sun. The laws modified the heliocentric theory of Nicolaus Copernicus, replacing its circular orbits and epicycles with elliptical trajectories, and explaining how planetary velocities vary. The three laws state that:
In astronomy, Kepler's laws of planetary motion, published by Johannes Kepler between 1609 and 1619, describe the orbits of planets around the Sun. The laws modified the heliocentric theory of Nicolaus Copernicus, replacing its circular orbits and epicycles with elliptical trajectories, and explaining how planetary velocities vary. The three laws state that:1.The orbit of a planet is an ellipse with the Sun at one of the two foci.
In astronomy, Kepler's laws of planetary motion, published by Johannes Kepler between 1609 and 1619, describe the orbits of planets around the Sun. The laws modified the heliocentric theory of Nicolaus Copernicus, replacing its circular orbits and epicycles with elliptical trajectories, and explaining how planetary velocities vary. The three laws state that:1.The orbit of a planet is an ellipse with the Sun at one of the two foci.2.A line segment joining a planet and the Sun sweeps out equal areas during equal intervals of time.
In astronomy, Kepler's laws of planetary motion, published by Johannes Kepler between 1609 and 1619, describe the orbits of planets around the Sun. The laws modified the heliocentric theory of Nicolaus Copernicus, replacing its circular orbits and epicycles with elliptical trajectories, and explaining how planetary velocities vary. The three laws state that:1.The orbit of a planet is an ellipse with the Sun at one of the two foci.2.A line segment joining a planet and the Sun sweeps out equal areas during equal intervals of time.3. The square of a planet's orbital period is proportional to the cube of the length of the semi-major axis of its orbit.
Answer:
They describe how
(1) planets move in elliptical orbits with the Sun as a focus,
(2) a planet covers the same area of space in the same amount of time no matter where it is in its orbit, and
(3) a planet's orbital period is proportional to the size of its orbit (its semi-major axis)
Explanation:
hope it helps you